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Volumn 338, Issue 6110, 2012, Pages 1047-1052

Making the moon from a fast-spinning earth: A giant impact followed by resonant despinning

Author keywords

[No Author keywords available]

Indexed keywords

ACCRETION; HYPOTHESIS TESTING; ISOTOPIC COMPOSITION; MANTLE; MOMENTUM; MOON; ORBITAL FORCING; RESONANCE;

EID: 84869779315     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1225542     Document Type: Article
Times cited : (555)

References (41)
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    • R. M. Canup, Icarus 168, 433 (2004).
    • (2004) Icarus , vol.168 , pp. 433
    • Canup, R.M.1
  • 11
    • 47149106054 scopus 로고    scopus 로고
    • R. M. Canup, Icarus 196, 518 (2008).
    • (2008) Icarus , vol.196 , pp. 518
    • Canup, R.M.1
  • 26
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    • Supplementary materials are available on
    • Supplementary materials are available on Science Online.
    • Science Online
  • 34
    • 84870988872 scopus 로고    scopus 로고
    • note
    • It is difficult to accurately calculate the mass of the atmosphere and the vapor fraction of the disk, as current numerical methods lack equations of state for multiple silicate phases in the mantle and multiphase flow of partially vaporized material (26). Although early work on the accretion of the Moon focused on a gas-poor disk (18, 25), recent studies indicate that the Moon may also accrete from a more vapor-rich atmosphere-disk structure (35, 36).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.